S. Cao

activity

20232026

most citedPSR B0943+10: Mode Switch, Polar Cap Geometry, and Orthogonally Polarized Radiation

11 citations · 30 across the 12 of their papers we have counts for

collaborators

Showing 2026Show all

4 papers · 1 filter

astro-ph.HE2026

Understanding Pulsar Magnetospheres with the SKAO

L. S. Oswald, A. Basu, M. Chakraborty +21

The SKA telescopes will bring unparalleled sensitivity across a broad radio band, a wide field of view across the Southern sky, and the capacity for sub-arraying, all of which make…

astro-ph.HE2026

Pulsar anti-glitches: starquakes driven by magnetism?

Hanyuan Long, Ruipeng Lu, Weiyang Wang +4

In the conventional starquake model of pulsar glitches, it is usually assumed that such events arise from fault slip induced by the self-gravity of compact objects. This inevitably…

astro-ph.HE2026

Constraining Pulsar Radiative Geometry via Multi-wavelength Modeling

Tong Zhao, Shunshun Cao, Renxin Xu

We propose that jointly modeling the thermal X-ray pulse profiles and the polarization position angles offers an effective means of locating the polarization orientation focus of t…

hep-ex2026

Search for proton decay via $p \to e^{+} π^{0} π^{0}$ and $p \to μ^{+} π^{0} π^{0}$ in 0.401 megaton-years exposure of Super-Kamiokande I-V

Kamiokande Collaboration, K. Abe, S. Abe +310

We searched for proton decay via $p \to e^{+} π^{0} π^{0}$ and $p \to μ^{+} π^{0} π^{0}$ in 0.401 megaton-years of data collected in all pure water detector phases of Super-Kamiokande…

Understanding Pulsar Magnetospheres with the SKAO

Pulsar anti-glitches: starquakes driven by magnetism?

Constraining Pulsar Radiative Geometry via Multi-wavelength Modeling

Search for proton decay via p→e+π0π0 and p→μ+π0π0 in 0.401 megaton-years exposure of Super-Kamiokande I-V

Search for proton decay via $p \to e^{+} π^{0} π^{0}$ and $p \to μ^{+} π^{0} π^{0}$ in 0.401 megaton-years exposure of Super-Kamiokande I-V